Spectral Characterization of Bennu Analogs Using PASCALE: A New Experimental Set-Up for Simulating the Near-Surface Conditions of Airless Bodies [0.03%]
基于PASCALE的新实验装置对小行星本努模拟样品的光谱特征研究
K L Donaldson Hanna,N E Bowles,T J Warren et al.
K L Donaldson Hanna et al.
We describe the capabilities, radiometric stability, and calibration of a custom vacuum environment chamber capable of simulating the near-surface conditions of airless bodies. Here we demonstrate the collection of spectral measurements of ...
Source-to-Sink Terrestrial Analogs for the Paleoenvironment of Gale Crater, Mars [0.03%]
火星盖尔陨石坑古环境的陆相类比研究：源到汇视角
Michael T Thorpe,Joel A Hurowitz,Kirsten L Siebach
Michael T Thorpe
In the Late Noachian to Early Hesperian period, rivers transported detritus from igneous source terrains to a downstream lake within Gale crater, creating a stratified stack of fluviolacustrine rocks that is currently exposed along the slop...
Jacob L Bean,Sean N Raymond,James E Owen
Jacob L Bean
Planets intermediate in size between the Earth and Neptune, and orbiting closer to their host stars than Mercury does the Sun, are the most common type of planet revealed by exoplanet surveys over the last quarter century. Results from NASA...
Evidence for a Diagenetic Origin of Vera Rubin Ridge, Gale Crater, Mars: Summary and Synthesis of Curiosity's Exploration Campaign [0.03%]
火星盖尔陨石坑弗雷娅·鲁宾 ridge 成岩以来改造的证据：好奇号探测任务成果总结与综合分析报告
A A Fraeman,L A Edgar,E B Rampe et al.
A A Fraeman et al.
This paper provides an overview of the Curiosity rover's exploration at Vera Rubin ridge (VRR) and summarizes the science results. VRR is a distinct geomorphic feature on lower Aeolis Mons (informally known as Mount Sharp) that was identifi...
Structure and composition of the distant lunar exosphere: Constraints from ARTEMIS observations of ion acceleration in time-varying fields [0.03%]
基于ARTEMIS观测的月球远端外层大气结构和组成：时变场中离子加速限制
J S Halekas,A R Poppe,W M Farrell et al.
J S Halekas et al.
By analyzing the trajectories of ionized constituents of the lunar exosphere in time-varying electromagnetic fields, we can place constraints on the composition, structure, and dynamics of the lunar exosphere. Heavy ions travel slower than ...
ARTEMIS observations of the solar wind proton scattering function from lunar crustal magnetic anomalies [0.03%]
月球 crust 磁异常对太阳风质子散射函数的 ARTEMIS 观测
A R Poppe,J S Halekas,C Lue et al.
A R Poppe et al.
Despite their small scales, lunar crustal magnetic fields are routinely associated with observations of reflected and/or backstreaming populations of solar wind protons. Solar wind proton reflection locally reduces the rate of space weather...
Edgard G Rivera-Valentín,Raina V Gough,Vincent F Chevrier et al.
Edgard G Rivera-Valentín et al.
The Mars Science Laboratory (MSL) Rover Environmental Monitoring Station (REMS) has now made continuous in situ meteorological measurements for several Martian years at Gale crater, Mars. Of importance in the search for liquid formation are...
Diagenesis of Vera Rubin Ridge, Gale Crater, Mars, From Mastcam Multispectral Images [0.03%]
火星盖尔陨石坑维拉·鲁宾岭的成岩作用:基于多光谱图像的研究
Briony H N Horgan,Jeffrey R Johnson,Abigail A Fraeman et al.
Briony H N Horgan et al.
Images from the Mars Science Laboratory (MSL) mission of lacustrine sedimentary rocks of Vera Rubin ridge on "Mt. Sharp" in Gale crater, Mars, have shown stark color variations from red to purple to gray. These color differences crosscut st...
Spectral, Compositional, and Physical Properties of the Upper Murray Formation and Vera Rubin Ridge, Gale Crater, Mars [0.03%]
火星盖尔陨石坑上部莫里站段和薇拉·鲁宾 ridge的光谱、成分及物理性质
S R Jacob,D F Wellington,J F Bell rd et al.
S R Jacob et al.
During 2018 and 2019, the Mars Science Laboratory Curiosity rover investigated the chemistry, morphology, and stratigraphy of Vera Rubin ridge (VRR). Using orbital data from the Compact Reconnaissance Imaging Spectrometer for Mars, scientis...
The Critical Point and the Supercritical State of Alkali Feldspars: Implications for the Behavior of the Crust During Impacts [0.03%]
碱长石的临界点和超临界状态：对撞击过程中地壳行为的意义
Anaïs Kobsch,Razvan Caracas
Anaïs Kobsch
The position of the vapor-liquid dome and of the critical point determine the evolution of the outermost parts of the protolunar disk during cooling and condensation after the Giant Impact. The parts of the disk in supercritical or liquid s...